| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.80 | 31.28 | 0.99 | 17.91 | 7.22 | 347.73 | -30.33 | 87.75 | 0.5027 | -433.3 | -330.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.41 | 0.00 | 1.87 | 7.01 | 352.33 | -25.73 | 88.46 | 0.4329 | -840.0 | -772.9 | |
| 1.80 | 2.33 | 0.99 | 1.28 | 7.03 | 352.12 | -25.94 | 88.41 | 0.4361 | -874.9 | -806.2 | |
| 0.00 | 1.53 | 0.00 | 0.84 | 8.18 | 351.64 | -26.42 | 85.75 | 0.4435 | -881.0 | -736.5 | |
| 0.00 | 0.90 | 0.00 | 0.50 | 7.78 | 350.91 | -27.15 | 86.66 | 0.4547 | -739.0 | -583.3 | |
| 0.00 | 1.35 | 0.00 | 0.75 | 7.16 | 350.64 | -27.42 | 88.02 | 0.4590 | -850.0 | -613.3 | |
| 0.00 | 1.71 | 0.00 | 0.96 | 7.25 | 349.53 | -28.53 | 87.77 | 0.4761 | -828.0 | -720.8 | |
| 0.00 | 1.80 | 0.00 | 1.03 | 6.93 | 347.87 | -30.19 | 88.31 | 0.5015 | -929.0 | -698.3 | |
| 0.00 | 2.87 | 0.00 | 1.65 | 6.76 | 347.45 | -30.61 | 88.63 | 0.5078 | -787.0 | -579.4 | |
| 0.00 | 1.89 | 0.00 | 1.08 | 6.94 | 347.44 | -30.62 | 88.27 | 0.5078 | -638.0 | -533.4 | |
| 0.00 | 1.35 | 0.00 | 0.77 | 6.57 | 347.32 | -30.73 | 88.99 | 0.5098 | -824.0 | -678.4 | |
| 0.00 | 1.80 | 0.00 | 1.04 | 6.52 | 347.01 | -31.05 | 89.06 | 0.5146 | -625.0 | -501.7 | |
| 0.00 | 1.08 | 0.00 | 0.63 | 7.51 | 345.38 | -32.68 | 87.07 | 0.5381 | -567.0 | -502.2 | |
| 0.00 | 1.35 | 0.00 | 0.79 | 6.18 | 345.05 | -33.01 | 89.50 | 0.5437 | -705.0 | -561.7 | |
| 0.00 | 1.17 | 0.00 | 0.69 | 6.66 | 345.01 | -33.05 | 88.61 | 0.5439 | -680.0 | -540.3 | |
| 0.00 | 2.25 | 0.00 | 1.34 | 8.27 | 344.03 | -34.03 | 85.64 | 0.5576 | 800.0 | 712.8 | |
| 0.00 | 0.72 | 0.00 | 0.43 | 6.23 | 344.02 | -34.04 | 89.30 | 0.5586 | 782.0 | 672.1 | |
| 0.00 | 2.87 | 0.00 | 1.72 | 8.16 | 343.78 | -34.28 | 85.83 | 0.5611 | 747.0 | 615.0 | |
| 0.00 | 0.90 | 0.00 | 0.54 | 8.21 | 343.14 | -34.92 | 85.74 | 0.5703 | 635.0 | 530.3 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |